Lebedev (lunar crater)
Lebedev is an impact crater on the far side of the Moon, lying at the eastern edge of the irregular mare feature known as Mare Australe and named for the Russian physicist Pëtr Nikolajevich Lebedev (1866–1912).1 The International Astronomical Union adopted the name in 1970, in the first wave of official names assigned to far-side features.1
| Key fact | Detail |
|---|---|
| Target and type | Moon, impact crater; IAU approval date 19701 |
| Diameter | 121.80 km per the IAU Gazetteer; some crater catalogs list 102 km1 |
| Center | 46.80° S, 107.89° E (planetographic, east positive); mapped on quad LAC-1171 |
| Eponym | Pëtr Nikolajevich Lebedev, Russian physicist (1866–1912)1 |
| Depth and volume | Depth about 2.9 km; rim rises about 1,490 m above the surroundings; volume roughly 10,400 km³2 |
| Satellite craters | Lebedev C, D, F, and K1 |
Location and surroundings
The crater sits in the southern hemisphere of the lunar far side, with its center at 46.80° S, 107.89° E and its extent running from 44.80° to 48.81° S and 104.95° to 110.82° E.1 It lies at the eastern edge of Mare Australe, southeast of the larger, lava-flooded crater Lamb and east-northeast of Anuchin, with the smaller crater Cassegrain to its southeast. A Russian-language crater description adds Pogson, Van der Waals, Pikelner, and Kugler among its neighbors.2
Physical appearance
Lebedev is a worn and eroded formation with an uneven outer rim, although no significant later impacts overlay the rim edge. A few small craterlets line the inner wall, a pair along the southeast and another to the southwest. The Russian description characterizes the crater as polygonal in outline, with a smoothed rim marked by many small craters, an inner slope that is narrowest in the north and widest in the southwest, and faint remnants of terraced structure on the western and eastern inner walls.2
Age
The Russian crater description assigns the formation of Lebedev itself to the pre-Nectarian period, the oldest division of the lunar geological time scale, and places the satellite crater Lebedev K in the Nectarian period.2
Satellite craters
By lunar mapping convention, satellite craters are identified by a letter placed on the side of the crater midpoint closest to the named feature.
| Satellite | Latitude | Longitude | Diameter |
|---|---|---|---|
| Lebedev C | 45.0° S | 111.0° E | 34 km |
| Lebedev D | 44.6° S | 112.5° E | 34 km |
| Lebedev F | 47.5° S | 110.8° E | 18 km |
| Lebedev K | 49.7° S | 108.9° E | 22 km |
Naming
The name honors Pëtr Nikolajevich Lebedev, a Russian physicist remembered for his experimental work on light pressure, and was approved by the IAU in 1970; the Gazetteer cites the World Who's Who in Science (edited by Allen G. Debus) as its reference for the biography.1 Far-side crater naming on this scale followed the program begun when an IAU Working Group on Lunar Nomenclature was appointed at the 1967 Prague meeting to assign names to features on the Moon's far side.3
Diameter discrepancy
The IAU Gazetteer gives a diameter of 121.80 km, while the crater catalog entry reproduced on several reference sites gives 102 km.1 The Gazetteer value is the one maintained by the USGS Astrogeology Science Center in cooperation with the IAU Working Group for Planetary System Nomenclature, the approving body for planetary names.4
References
- Gazetteer of Planetary Nomenclature, Feature 3320: Lebedev, USGS Astrogeology
- Лебедев (лунный кратер), agro-archive.ru
- Introduction to far-side nomenclature, NASA Technical Reports Server
- Gazetteer of Planetary Nomenclature, USGS
Topic: Encyclopedia › Places and geography › Extraterrestrial places › Planetary surfaces and named features › Lunar surface features › Lunar craters › Far-side and limb lunar craters › Far-side southern-hemisphere craters
Initially written Oct 21, 2026 · Edited: Oct 25, 2026
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